Numerical simulations of type I planetary migration in nonturbulent magnetized discs
Using 2D MHD numerical simulations performed with two different finite difference Eulerian codes, we analyze the effect that a toroidal magnetic field has on low mass planet migration in nonturbulent protoplanetary discs. The presence of the magnetic field modifies the waves that can propagate in th...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2005
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